首页 | 本学科首页   官方微博 | 高级检索  
     


Orbital periods of cataclysmic variables identified by the SDSS – III. Time-series photometry obtained during the 2004/5 International Time Project on La Palma
Authors:M. Dillon,B. T. Gä  nsicke,A. Aungwerojwit,P. Rodrí  guez-Gil,T. R. Marsh,S. C. C. Barros,P. Szkody,S. Brady,T. Krajci, A. Oksanen
Affiliation:Department of Physics, University of Warwick, Coventry CV4 7AL;Department of Physics, Faculty of Science, Naresuan University, Phitsanulok 65000, Thailand;Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain;Department of Astronomy, University of Washington, Seattle, WA 98195, USA;5 Melba Drive, Hudson, NH 03051, USA;Astrokolkhoz Observatory, PO Box 1351 Cloudcroft, NM 88317, USA;Hankasalmi Observatory, Kyllikinkatu 1, FI-40100 Jyväskylä, Finland
Abstract:
Keywords:binaries: close    binaries: eclipsing    binaries: spectroscopic    stars: dwarf novae    novae, cataclysmic variables    white dwarfs
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号